Gamma-Ray Burst Follow-up Observations with STACEE During 2003-2007

Details Gamma-Ray Burst Follow-up Observations with STACEE During 2003-2007 Gamma-Ray Burst Follow-up Observations with STACEE During 2003-2007

2007-10-22

arxiv.org/abs/0710.4149v1

Astronomy and Astrophysics

Astrophysics

4 pages, 1 table, 2 figures, presented at the 30th International Cosmic Ray Conference, Merida, Mexico, 2007

Scientific paper

The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) is an atmospheric Cherenkov telescope (ACT) that uses a large mirror array to achieve a relatively low energy threshold. For sources with Crab-like spectra, at high elevations, the detector response peaks near 100 GeV. Gamma-ray burst (GRB) observations have been a high priority for the STACEE collaboration since the inception of the experiment. We present the results of 20 GRB follow-up observations at times ranging from 3 minutes to 15 hours after the burst triggers. Where redshift measurements are available, we place constraints on the intrinsic high-energy spectra of the bursts.

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